PASTORELLO, AndreaAndreaPASTORELLO0000-0002-9719-3157Wyrzykowski, L.L.Wyrzykowski0000-0002-3256-0016Valenti, S.S.Valenti0000-0001-5008-8619Prieto, J. L.J. L.Prieto0000-0002-1381-9125Kozlowski, S.S.Kozlowski0000-0002-7259-4624Udalski, A.A.Udalski0000-0002-3938-692XELIAS DE LA ROSA, NANCY DEL CARMENNANCY DEL CARMENELIAS DE LA ROSAMorales-Garoffolo, A.A.Morales-GaroffoloAnderson, J. P.J. P.AndersonBenetti, S.S.BenettiBersten, M.M.BerstenBOTTICELLA, MARIA TERESAMARIA TERESABOTTICELLACAPPELLARO, EnricoEnricoCAPPELLAROFasano, G.G.FasanoFraser, M.M.FraserGal-Yam, A.A.Gal-YamGillone, M.M.GilloneGraham, M. L.M. L.GrahamGreiner, J.J.GreinerHachinger, S.S.HachingerHowell, D. A.D. A.HowellInserra, C.C.InserraParrent, J.J.ParrentRau, A.A.RauSchulze, S.S.SchulzeSmartt, S. J.S. J.SmarttSmith, K. W.K. W.SmithTURATTO, MassimoMassimoTURATTOYaron, O.O.YaronYoung, D. R.D. R.YoungKubiak, M.M.KubiakSzymanski, M. K.M. K.SzymanskiPietrzynski, G.G.PietrzynskiSoszynski, I.I.SoszynskiUlaczyk, K.K.UlaczykPoleski, R.R.PoleskiPietrukowicz, P.P.PietrukowiczSkowron, J.J.SkowronMroz, P.P.Mroz2020-08-192020-08-192017http://hdl.handle.net/20.500.12386/26711Photometric measurements in the optical and NIR bands were obtained through the PSF-fitting technique. A template PSF was built using stars in the SN field. With this PSF model along with a low-order polynomial surface, we finally performed a fit to the SN and the underlying background. OGLE-IV photometry was obtained using the difference imaging analysis, which is a template subtraction method adapted to the OGLE data and detailed in Wyrzykowski et al. 2014, J/AcA/64/197 (see also Wozniak 2000, J/AcA/50/421). <P />(2 data files). <P />enDatabasehttps://cdsarc.unistra.fr/viz-bin/cat/J/MNRAS/449/19412017yCat..74491941PFIS/05 - ASTRONOMIA E ASTROFISICA